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Chandra, NICER, Swift, Hubble, and TESS have produced rich multiwavelength data sets of stellar time-variability and X-ray and ultraviolet emission that can inform our understanding of stars and provide
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to study biophysical forcing and interactions between radiation and variations in ocean biological and physical fields. Applicants should have experience in mathematical/statistical methods, data analysis
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of the United States. A complete list of Designated Countries can be found at: https://www.nasa.gov/oiir/export-control . Eligibility is currently open to: U.S. Citizens; U.S. Lawful Permanent Residents (LPR); Foreign
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missions, including data from NASA's Kepler mission, the James Webb Space Telescope, and future coronagraphic and transiting exoplanet missions. Finally, Ames is putting significant effort into developing a
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critical constraints on physical models of SEEs. This opportunity has a particular focus on data from the Hinode EUV Imaging Spectrometer: identifying key datasets from the 18-year mission; performing plasma
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capability of CMEs, as derived from the interplanetary radio emission associated with these solar eruptions. Spacecraft data obtained by white-light coronagraphs and radio instruments are used
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experience in the planetary science literature will be more suitable for this research opportunity. Additional benefit would be provided by past experience with planetary image datasets, data science tools
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). Revisiting Ionosphere-Thermosphere Responses to Solar Wind Driving in Superstorms of November 2003 and 2004. J. Geophys. Res., 122. https://doi.org/10.1002/2017JA024542 . 2. McGranaghan, R. M., A. J. Mannucci